Dusty Structure Around Type 1 AGNs
Abstract
We present a detailed investigation of the MIR continuum emission of type 1 QSOs and define the main emission components. Our model requires three components: a clumpy torus, dusty narrow-line region (NLR) clouds and a blackbody-like hot dust.
- Publication:
-
Co-Evolution of Central Black Holes and Galaxies
- Pub Date:
- May 2010
- DOI:
- 10.1017/S1743921310005867
- Bibcode:
- 2010IAUS..267..125M
- Keywords:
-
- galaxies: active;
- quasars: general